"We are so ignorant about the abiotic processes in the atmosphere that we cannot immediately exclude the claims that life exists today." -Joseph O'Rourke
One of the most painful things about Venus news is that even in LPI's, the speaker usually wastes a lot of time before getting to anything good. There's the rub though. If we knew jack about Venus the phosphine discovery would have been easily confirmable or disprovable. Thus we need to know more no matter what. This one does not start to go over anything interesting till 20:00. Starting slow and ending on a flurry of good stuff is pretty normal, and here we go.
- At 20:00 he's got a nice slide mapping two varieties of crater and volcano distribution. We've all seen the random distribution of craters dating Venus surface before, but this slide has a subdivision by implying pristine craters are younger than those that are infilled.
- At 26:55 he starts getting into counterarguments about a stagnant-lid. He shows beautiful slides noting possible subduction. He will return to this idea when wrapping up.
- At 39:37 there's a great slide showing a current hypothesis, the "squishy-lid" as opposed to a stagnant-lid.
- The big reveal he saves for the end involves a possibility of a Basal Magma Ocean (BMO). The implications are pretty huge. If Venus lithosphere is floating, it follows physics more like Titan than Earth. And there are more dynamo possibilities. This is why he titles his lecture as he did. If a BMO then Venus is cooling slower than Earth, if not... then Venus should behave more Earth-like.
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